On the Relation Between Coronal Green Line Brightness and Magnetic Fields Intensity

Journal article

Peer reviewed

Xue-Fei Zhang, Yu Liu, Ming-Yu Zhao, Teng-Fei Song, Jing-Xing Wang, Xiao-Bo Li and Zi-Han Li

Research in astronomy and astrophysics, Vol.22(7), p.75007

01/07/2022

Abstract

Stars: coronae

Sun: activity

Sun: atmosphere

Sun: corona

Sun: coronal mass ejections (CMEs)

Sun: fundamental parameters

Sun: heliosphere

Sun: magnetic fields

Sun: UV radiation

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Title: On the Relation Between Coronal Green Line Brightness and Magnetic Fields Intensity
Creators - without role: Xue-Fei Zhang - University of Chinese Academy of Sciences , Beijing 100049, China
Yu Liu - Yunnan Normal University
Ming-Yu Zhao - Yunnan Observatories
Teng-Fei Song - University of Chinese Academy of Sciences , Beijing 100049, China
Jing-Xing Wang - Yunnan Observatories
Xiao-Bo Li - Yunnan Observatories
Zi-Han Li - Yunnan Normal University
Publication Details: Research in astronomy and astrophysics, Vol.22(7), p.75007
Publisher: National Astromonical Observatories, CAS and IOP Publishing
Number of pages: 11
Identifiers: 9950084908331
Academic Unit: King Saud University
Language: English
Resource Type: Journal article